Hammond, G. , Hild, S. and Pitkin, M. (2014) Advanced technologies for future ground-based, laser-interferometric gravitational wave detectors. Journal of Modern Optics, 61(Sup. 1), S10-S45. (doi: 10.1080/09500340.2014.920934) (PMID:25705087) (PMCID:PMC4311950)
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91589.pdf - Published Version Available under License Creative Commons Attribution. 2MB |
Publisher's URL: http://dx.doi.org/10.1080/09500340.2014.920934
Abstract
We present a review of modern optical techniques being used and developed for the field of gravitational wave detection. We describe the current state-of-the-art of gravitational waves detector technologies with regard to optical layouts, suspensions and test masses. We discuss the dominant sources and noise in each of these subsystems and the developments that will help mitigate them for future generations of detectors. We very briefly summarise some of the novel astrophysics that will be possible with these upgraded detectors.
Item Type: | Articles |
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Status: | Published |
Refereed: | Yes |
Glasgow Author(s) Enlighten ID: | Hammond, Professor Giles and Hild, Professor Stefan and Pitkin, Dr Matthew |
Authors: | Hammond, G., Hild, S., and Pitkin, M. |
Subjects: | Q Science > QB Astronomy Q Science > QC Physics |
College/School: | College of Science and Engineering > School of Physics and Astronomy |
Research Centre: | College of Science and Engineering > School of Physics and Astronomy > Institute for Gravitational Research |
Journal Name: | Journal of Modern Optics |
Publisher: | Taylor & Francis |
ISSN: | 0950-0340 |
ISSN (Online): | 1362-3044 |
Copyright Holders: | Copyright © 2014 The Authors |
First Published: | First published in Journal of Modern Optics 61(Sup.1):S10-S45 |
Publisher Policy: | Reproduced under a Creative Commons License |
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